Abstract
We have used archival ROSAT data to present X-ray images of 31 supernova remnants (SNRs) in the Large Magellanic Cloud (LMC). We have classified these remnants according to their X-ray morphologies, into the categories of shell-type, diffuse face, centrally brightened, point-source-dominated, and irregular. We suggest possible causes of the X-ray emission for each category and for individual features of some of the SNRs.
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CITATION STYLE
Williams, R. M., Chu, Y., Dickel, J. R., Petre, R., Smith, R. C., & Tavarez, M. (1999). Supernova Remnants in the Magellanic Clouds. III. An X‐Ray Atlas of Large Magellanic Cloud Supernova Remnants. The Astrophysical Journal Supplement Series, 123(2), 467–485. https://doi.org/10.1086/313246
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